Paper
7 May 2009 The flying mirror: future brightest x-ray and γ-ray source
T. Zh. Esirkepov, S. V. Bulanov, M. Kando, A. S. Pirozhkov, A. G. Zhidkov
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Abstract
An ultra-bright high-power X-ray and γ-ray source is proposed. A relativistic flying mirror reflects a counterpropagating electromagnetic radiation causing its frequency multiplication and intensification, while the role of the mirror is played by a solid-density thin plasma slab accelerating in the radiation pressure dominant regime. Frequencies of high harmonics generated at the flying mirror by a relativistically strong counter-propagating radiation undergo multiplication with the same factor as the fundamental frequency of the reflected radiation, approximately equal to the quadruple of the square of the mirror Lorentz factor. The theory of the reflectivity of a moving thin plasma slab is presented.
© (2009) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
T. Zh. Esirkepov, S. V. Bulanov, M. Kando, A. S. Pirozhkov, and A. G. Zhidkov "The flying mirror: future brightest x-ray and γ-ray source", Proc. SPIE 7359, Harnessing Relativistic Plasma Waves as Novel Radiation Sources from Terahertz to X-Rays and Beyond, 735909 (7 May 2009); https://doi.org/10.1117/12.820615
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CITATIONS
Cited by 2 scholarly publications.
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KEYWORDS
Mirrors

Plasma

X-rays

Electromagnetic radiation

Ions

Gamma radiation

Pulsed laser operation

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